X-Ray and Gamma-Ray Emissions from the PSR 1259$-$63/Be Star System
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/55/2/473/6022891/pasj55-0473.pdf
Reference25 articles.
1. Probing pulsar winds using inverse Compton scattering
2. Bremsstrahlung, Synchrotron Radiation, and Compton Scattering of High-Energy Electrons Traversing Dilute Gases
3. Very-high-energy gamma radiation associated with the unshocked wind of the Crab pulsar
4. Non-pulsed gamma radiation from a binary system with a pulsar
5. Detection of X-ray emission from the PSR 1259-63/SS 2883 binary system
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1. Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind;Monthly Notices of the Royal Astronomical Society;2019-10-07
2. Modelling multiwavelength emissions from PSR B1259–63/LS 2883: Effects of the stellar disc on shock radiations;Astronomy & Astrophysics;2019-07
3. Evidence on the Orbital Modulated Gamma-Ray Emissions from the Redback Candidate 3FGL J2039.6–5618;The Astrophysical Journal;2018-11-02
4. Hydrodynamic Interaction between the Be Star and the Pulsar in the TeV Binary PSR B1259$-$63/LS 2883;Publications of the Astronomical Society of Japan;2011-08-25
5. SUZAKUOBSERVATIONS OF PSR B1259–63: A NEW MANIFESTATION OF RELATIVISTIC PULSAR WIND;The Astrophysical Journal;2009-05-26
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